\begin{table}%t3  
\caption{Spots configuration for IM~Peg.  The stellar parameters used in the solution are:
unspotted effective temperature, $T_{\rm max}$~= 4666~K; limb-darkening coefficients at~$V$ and
at 6200~\AA, $\mu_{\rm V}$~= 0.80, $\mu_{6200}$~= 0.68; inclination, $i$~= 60$^{\circ}$.}
\label{tab:parameters_im}
%\centering
\par
\begin{tabular}{llcrccc}
\hline
\hline
 \noalign{\smallskip}
 Model   &  Radius  &  Lon.  &   Lat.  &  $\frac{T_{\rm sp}}{T_{\rm ph}}$ &
  $A_{\rm rel}$ \\ 
 \noalign{\smallskip}
\hline
 Planck   & 27$\fdg$2	&  123$\degr$  &  138$\degr$  &  0.873 $\pm$ 0.050  &  0.093 $\pm$ 0.025   \\
  "  "    & 21$\fdg$8	&  223$\degr$  &  149$\degr$  &  0.873 $\pm$ 0.050  &      \\
 Kurucz   & 28$\fdg$5	&  123$\degr$  &  138$\degr$  &  0.904 $\pm$ 0.027  &  0.106 $\pm$ 0.020   \\
  "  "    & 23$\fdg$4	&  223$\degr$  &  149$\degr$  &  0.904 $\pm$ 0.027  &	      \\
 NextG    & 30$\fdg$0  &  123$\degr$  &  138$\degr$  &   0.915 $\pm$ 0.030   &   0.115 $\pm$ 0.030 	\\
  "  "    & 23$\fdg$9  &  223$\degr$  &  149$\degr$  &   0.915 $\pm$ 0.030   &       \\
\hline
\end{tabular}
\end{table}